With the latest observations from the Planck satellite, researchers from the Niels Bohr Institute, among others, may be closer than ever to a solution to the origin of the mysterious dark matter.

With the latest observations from the Planck satellite, researchers from the Niels Bohr Institute, among others, may be closer than ever to a solution to the origin of the mysterious dark matter.The universe is comprised of a large amount of invisible matter, dark matter.It fills the space between the galaxies and between the stars in the galaxies. Since the prediction of the existence of dark matter more than 70 years ago, all sorts of researchers -- astronomers, cosmologists and particle physicists -- have been looking for answers to what it could be.

The Planck satellite, which was launched in 2009, has extremely sensitive instruments that can map microwave radiation in the entire sky with great precision. The latest data from the Planck mission reveals unusual radiation from our own galaxy, which open a new direction in understanding the most fundamental properties of the space, time and matter in the universe.

“We have observed a very unique emission of radio radiation from the center of our galaxy, the Milky Way,” explained Pavel Naselsky, professor of cosmology at the Discovery Center at the Niels Bohr Institute at the University of Copenhagen.

“By using different methods to separate the signal for very broad range of wavelengths, we have been able to determine the spectrum of the radiation. The radiation originates from synchrotron emission, i.e., electrons and positrons circulating at high energies around the lines of the magnetic field in the center of the galaxy, and there are quite strong indications that it could come from dark matter,” said Naselsky.

Naselsky explains that leading scientists like Niels Bohr professor Subir Sarkar have predicted, using calculations, that dark matter may consist of very heavy particles that are around 10 times as heavy as the Higgs particle, that is to say, 1,000 times heavier than a proton. But they have very unique properties and do not interact with ‘normal’ matter particles. Dark matter particles are also usually very scattered and do not interact with each other.

“But we know from theoretical predictions that the concentration of dark matter particles around the center of galaxies is very high and we have a strong argument they can collide there and in the collision electrons and positrons are formed. These electrons and positrons start to rotate around the magnetic field at the center of the galaxy and in doing so produce this very unusual synchrotron radiation,” stated Naselsky.

It has simply not been possible to observe this radiation in such detail before, as previous instruments have not been sensitive enough. But with Planck, this unusual radiation is seen very clearly.

“The radiation cannot be explained by the structural mechanisms in the galaxy and it cannot be radiation from supernova explosions. We believe that this could be proof of dark matter. Otherwise, we have discovered absolutely new (and unknown for physics) mechanism of acceleration of particles in the galactic center,” he added.

Naselsky expects exciting new results may come within the next few months.